Description of AESFAST This model is based on a physical formulation of transmittance, namely the Goody random model. It can therefore work on any vertical coordinate (as opposed to fixed pressure levels). It is presented in Garand et al, 1999. The model considers up to 8 gases. The forward model is accompanied by an analytic Jacobian routine. Jacobians for temperature and each of the 8 gases are available (most fast models compute only T, H2O and O3 Jacobians). It can be used in data assimilation for NWP models. The Goody formulation is used for 6 gases: H2O, CO2, O3, CO, CH4 and N2O. Continua for H2O, O2 and N2 are also considered. The optical depths of each gas is multiplied by an adjustment factor, typically closed to unity, for a global fit to LBL transmittances available from an ensemble of 189 profiles. The most dominant gas in the channel is adjusted last in such a way as to minimize the errors in terms of resulting brightness temperature considering all gases. The procedure to establish adjustment factors is fully automated, allowing quick adaptation to new sets of HIRS-like channels. The model is designed for infrared channels only (no scattering). It allows variable surface emissivity. Cloudy atmospheres can be treated as well with the effective cloud amount provided in each layer as input. Garand, L., D. S. Turner, C. Chouinard, and J. Halle, 1999. A physical formulation of atmospheric transmittance for the massive assimilation of satellite infrared radiances. J. Appl. Meteor., 38, 541-554. Description of AESFAST2 This is the same model as AESFAST, except that the Goody random formulation of transmittance is now supplemented by an additional dependency on pressure for the mean line width. This dependency is of the form (1. + c P/Po) where c is the adjustment factor, P is the pressure of the layer and Po is a reference pressure. This new adjustment provided a very large improvement in HIRS-02 (for CO2) and a significant improvement in HIRS-09 (for O3). The minimization procedure to find “c” is straightforward but we find in practice that the end result may be influenced by the initial choice of c in some channels. With the evolution to narrow channels, it is preferable to pre-determine, if possible, areas where the original AESFAST can best work.